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This middle panel of this plot shows the fit (red curve) to the
observed pulseshape (black curve) for the star G29-38; this fit is
achieved by varying the convective parameters, the amplitude and
phase of the mode, and the inclination angle. In the upper panel,
we see that the derived thermal response timescale of the
convection zone (red curve) is very similar to that which one
calculates from standard mixing-length theory (black curve). For a
movie of this solution, click here.